Hα observations of Be stars | Astron. Astrophys. Suppl. Ser.

Free access article

Issue		Astron. Astrophys. Suppl. Ser. Volume 147, Number 2, December I 2000


Page(s)		229 - 242
DOI		http://dx.doi.org/10.1051/aas:2000299

DOI: 10.1051/aas:2000299

Astron. Astrophys. Suppl. Ser. 147, 229-242

H $\alpha$ observations of Be stars

D.P.K. Banerjee - S.D. Rawat - P. Janardhan

Send offprint request: D.P.K. Banerjee,
e-mail: orion@prl.ernet.in

Astronomy and Astrophysics Division, Physical Research Laboratory, Navrangpura, Ahmedabad 380 009, India

Received May 22; accepted September 11, 2000

Abstract:

We present here the H $\alpha$ spectra of 44 Be stars taken at a resolution of 0.5 Å. From the spectra, different emission line parameters have been deduced. A study of the correlations between different pairs of these parameters has been made with a view to understanding the mechanisms of line formation and shaping in Be stars.

Key words: Be stars -- spectroscopy -- line profiles

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H observations of Be stars

Abstract:

H $\alpha$ observations of Be stars